3.Reconstruction of Coronal Field

	To understand the flare/CME process, we applied Yan & Sakurai(2000:Solar Phys.,v195, 89-109) non-constant-a force-free field model
	to reconstruct
	the 3d field
	in corona

 

Responsible NASA Official:  Gordon D. Holman Web Design:  Merrick Berg, Brian Dennis, Gordon Holman, & Gilbert Prevost Heliophysics Science Division NASA/Goddard Space Flight Center Laboratory for Solar Physics/ Code 671 Greenbelt, MD, 20771, USA Gordon.D.Holman@nasa.gov

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